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search results for `Watson A A` |u:people.ast.cam.ac.uk
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https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt2 Jul 2010: Since, as noted before, a sensible observing sequence precludes it being a problem. ... There has been a further shrinkage of staff at UKIRT. Tom Kerr is now our main contact with Watson the other UKIRT contact. -
arX iv:1 008. 0865 v2 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/cws10.pdf22 Aug 2010: This was then subtracted from the final. image to ensure a flat background. ... 2006), compared to a belt at 55AU with a width of50AU for HD191089. -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: Weshow that there is no significant statistical difference between fractional excessesof A-stars. ... 5). We also assume that the central star acts like a black-body. -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: possibilitiesinclude dynamical scattering by a migrating planet, see e.g.Gomes et al. ... This source together with HD 31295 andHD 38206 are described in Appendix A.
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